Distribution and Anisotropy of the Energy Transfer Rate in the Solar Wind Turbulence
The distribution of the energy transfer rate is critical for the interpretation of the intermittent energy cascade in the solar wind turbulence. However, the true observational distribution of the energy transfer rate in the solar wind and its anisotropy
Honghong Wu +4 more
doaj +1 more source
Observations of 1/f Noise at Mercury’s Solar Wind Using MESSENGER Data
Low-frequency signals having a band-limited scale-invariant power, or “1/ f ” noise, have been detected in the interplanetary medium and inferred from coronal and photospheric observations.
Rayta A. Pradata +6 more
doaj +1 more source
Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets [PDF]
A computational model for the determination of the detailed plasma and magnetic field properties of the global interaction of the solar wind with nonmagnetic terrestrial planetary obstacles is described.
Spreiter, J. R., Stahara, S. S.
core +1 more source
We present a first record of significantly enhanced occurrences of magnetic reconnection exhausts as measured by the Wind satellite across a stream interaction region (SIR) at 1 au from 2019 January 4 10:11:20 UT to 2019 January 5 09:58:00 UT.
S. Eriksson +3 more
doaj +1 more source
Solar and interplanetary magnetic fields and plasmas [PDF]
Recent observations of solar and interplanetary magnetic fields and ...
Wilcox, J. M.
core +1 more source
Upstream IMF Influence on Closed Magnetic Field Orientation on Mars
Closed magnetic fields play an important role in plasma transport and atmospheric escape from the Martian dayside ionosphere. Leveraging in‐situ magnetic field data from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, we conduct a statistical
JunFeng Qin +5 more
doaj +1 more source
Large-scale interplanetary magnetic fields: Voyager 1 and 2 observations between 1 AU and 9.5 AU [PDF]
The large-scale radial and temporal variations of the interplanetary magnetic field strength B observed by Voyagers 1 and 2 are discussed. Two components of the magnetic field strength were considered: (1) an average component, B sub zero, based on solar
Behannon, K. W. +3 more
core +1 more source
Electrodynamic forcing of the Duskside ionosphere and the super fountain effect during the superstorm of May 10 to 11 2024. [PDF]
Venugopal I, Thampi SV, Bhaskar A.
europepmc +1 more source
Europa Clipper Magnetometer Boom Deployment: A First Look at the Magnetometer Observations of the Spacecraft and the Interplanetary Magnetic Field. [PDF]
Cochrane CJ +21 more
europepmc +1 more source
IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]
Cohen CMS +30 more
europepmc +1 more source

